129 research outputs found
The Complex Upper HR Diagram
Several decades of observations of the most massive and most luminous stars
have revealed a complex upper HR Diagram, shaped by mass loss, and inhabited by
a variety of evolved stars exhibiting the consequences of their mass loss
histories. This review presents a brief historical overview of the HR Diagram
for massive stars, highlighting some of the primary discoveries and results
from their observation in nearby galaxies. The chapters in this volume include
reviews of our current understanding of different groups of evolved massive
stars, all losing mass and in different stages of their evolution; the Luminous
Blue Variables (LBVs), B[e] supergiants, the warm hypergiants, Wolf-Rayet
stars, and the population of OB stars and supergiants in the Magellanic Clouds.Comment: Introductory review chapter for e-book "Luminous stars in Nearby
Galaxies" (https://www.mdpi.com/journal/galaxies/special_issues/Luminous
Incorporating the APS Catalog of the POSS I and Image Archive in ADS
The primary purpose of this contract was to develop the software to both create and access an on-line database of images from digital scans of the Palomar Sky Survey. This required modifying our DBMS (called Star Base) to create an image database from the actual raw pixel data from the scans. The digitized images are processed into a set of coordinate-reference index and pixel files that are stored in run-length files, thus achieving an efficient lossless compression. For efficiency and ease of referencing, each digitized POSS I plate is then divided into 900 subplates. Our custom DBMS maps each query into the corresponding POSS plate(s) and subplate(s). All images from the appropriate subplates are retrieved from disk with byte-offsets taken from the index files. These are assembled on-the-fly into a GIF image file for browser display, and a FITS format image file for retrieval. The FITS images have a pixel size of 0.33 arcseconds. The FITS header contains astrometric and photometric information. This method keeps the disk requirements manageable while allowing for future improvements. When complete, the APS Image Database will contain over 130 Gb of data. A set of web pages query forms are available on-line, as well as an on-line tutorial and documentation. The database is distributed to the Internet by a high-speed SGI server and a high-bandwidth disk system. URL is http://aps.umn.edu/IDB/. The image database software is written in perl and C and has been compiled on SGI computers with MIX5.3. A copy of the written documentation is included and the software is on the accompanying exabyte tape
- …